1  12.00  H 
 2  10.78  He
 3   1.36  Li
 4   1.66  Be
 5   3.03  B 
 6   8.35  C 
 7   7.71  N 
 8   8.61  O 
 9   4.41  F 
10   7.90  Ne
11   6.62  Na
12   7.87  Mg
13   6.79  Al
14   7.86  Si
15   5.49  P 
16   7.23  S 
17   5.10  Cl
18   6.35  Ar
19   5.44  K 
20   6.64  Ca
21   3.43  Sc
22   5.26  Ti
23   4.33  V 
24   5.98  Cr
25   5.70  Mn
26   7.85  Fe
27   5.25  Co
28   6.55  Ni
29   4.54  Cu
30   4.92  Zn
 -1
%filename: sun_coronal_2012_schmelz_ext.abund
%created for the CHIANTI atomic database by Peter Young, 11-Dec-2015
%abundance: 
   Schmelz, J.T., Reames, D.V., von Steiger, R., & Basu, S. 2012, ApJ, 755, 33
         <bibcode="2012ApJ...755...33S">
   Caffau, E., Ludwig, H.-G., Steffen, M., Freytag, B. & Bonifacio, P. 2011, Sol. Phys.
         268, 255  <bibcode="2011SoPh..268..255C">
   Lodders, K., Palme, H., & Gail, H.P. 2009, Astronomy, Astrophysics, and Cosmology, B:
         Solar System, Landolt-Bornstein, New Series VI/4, Spring, Berlin, 560
         <bibcode="2009LanB...4B...44L">
%comment:
   This file reproduces the abundances from the file sun_coronal_2012_schmelz.abund but
   adds in values for the elements missing in this file. For these missing elements, the
   photospheric abundances are taken from the sun_photospheric_2011_caffau.abund and
   then multiplied by a scaling factor. The scaling factor comes from Schmelz et al.
   (2012) and is 2.14 below FIP=9 eV, 0.71 above FIP=11 eV, and a linearly varying
   factor between these two energies.
 -1